We report on the implications for cosmic inflation of the 2018 release of the Planck cosmic
microwave background (CMB) anisotropy measurements. The results are fully consistent …

We present a new model of interstellar dust in which large grains are a single composite
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …

The study of polarized dust emission has become entwined with the analysis of the cosmic
microwave background (CMB) polarization in the quest for the curl-like B-mode polarization …

We present a synthesis of the astronomical observations constraining the wavelength-
dependent extinction, emission, and polarization from interstellar dust from UV to microwave …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …

The dielectric function of interstellar dust material is modeled using observations of
extinction and polarization in the infrared, together with estimates for the mass of interstellar …

We present synthetic dust polarization maps of simulated molecular clouds with the goal to
systematically explore the origin of the relative orientation of the magnetic field () with …

In this white paper we introduce the IMAGINE Consortium and its scientific background,
goals and structure. The purpose of the consortium is to coordinate and facilitate the efforts …

Accurate characterization of the polarized dust emission from our Galaxy will be decisive in
the quest for the cosmic microwave background (CMB) primordial B-modes. An incomplete …